{"title":"在 $f(R)$ 引力下修正黑洞度量的热力学特性","authors":"Wen-Xiang Chen, Yao-Guang Zheng","doi":"arxiv-2405.14894","DOIUrl":null,"url":null,"abstract":"To construct new Schwarzschild and Kerr-Newman metric solutions, we start\nfrom the Lagrangian in entropy and statistical mechanics, introducing $f(R)$\ngravity theory and dark energy definitions. Through a series of calculations,\nwe derive the corrected metric solutions under different forms of $f(R)$\ngravity.","PeriodicalId":501190,"journal":{"name":"arXiv - PHYS - General Physics","volume":"39 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-05-21","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Thermodynamic Properties of Modified Black Hole Metrics in $f(R)$ Gravity\",\"authors\":\"Wen-Xiang Chen, Yao-Guang Zheng\",\"doi\":\"arxiv-2405.14894\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"To construct new Schwarzschild and Kerr-Newman metric solutions, we start\\nfrom the Lagrangian in entropy and statistical mechanics, introducing $f(R)$\\ngravity theory and dark energy definitions. Through a series of calculations,\\nwe derive the corrected metric solutions under different forms of $f(R)$\\ngravity.\",\"PeriodicalId\":501190,\"journal\":{\"name\":\"arXiv - PHYS - General Physics\",\"volume\":\"39 1\",\"pages\":\"\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2024-05-21\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"arXiv - PHYS - General Physics\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/arxiv-2405.14894\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"arXiv - PHYS - General Physics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/arxiv-2405.14894","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Thermodynamic Properties of Modified Black Hole Metrics in $f(R)$ Gravity
To construct new Schwarzschild and Kerr-Newman metric solutions, we start
from the Lagrangian in entropy and statistical mechanics, introducing $f(R)$
gravity theory and dark energy definitions. Through a series of calculations,
we derive the corrected metric solutions under different forms of $f(R)$
gravity.
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